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The Next Generation Fornax Survey (NGFS). IV. Mass and Age Bimodality of Nuclear Clusters in the Fornax Core Region

  • Authors: Yasna Ordenes-Briceño, Thomas H. Puzia, Paul Eigenthaler, Matthew A. Taylor, Roberto P. Muñoz, Hongxin Zhang, Karla Alamo-Martínez, Karen X. Ribbeck, Eva K. Grebel, Simón Ángel, Patrick Côté, Laura Ferrarese, Michael Hilker, Ariane Lançon, Steffen Mieske, Bryan W. Miller, Yu Rong, and Ruben Sánchez-Janssen

2018 The Astrophysical Journal 860 4.

  • Provider: AAS Journals

Caption: Figure 4.

Illustration of the galaxy fitting for two dwarf galaxies in the three optical bands, ﹩u^{\prime} g^{\prime} i^{\prime} ﹩ from left to right, respectively. The top row shows the original image, and the bottom row shows the best residual images (GALAXY—MODEL), where the nuclear star cluster is deliberately left in the center and is visible in all filters. A scale bar (solid line) is shown at the bottom left image corresponding to ﹩10\buildrel{\prime\prime}\over{.} 3\,\hat{=}1\,\mathrm{kpc}﹩.

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